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Theory of interacting Bose and Fermi gases in traps

Crete, July 2007 Summer School on Bose-Einstein Condensation. Theory of interacting Bose and Fermi gases in traps. Sandro Stringari. 2nd lecture. Dynamics of superfluids. University of Trento. CNR-INFM. Understanding superfluid features requires theory for transport phenomena

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Theory of interacting Bose and Fermi gases in traps

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  1. Crete, July 2007 Summer School on Bose-Einstein Condensation Theory of interacting Bose and Fermi gases in traps Sandro Stringari 2nd lecture Dynamics of superfluids University of Trento CNR-INFM

  2. Understanding superfluid features requires theory for transport phenomena (crucial interplay between dynamics and superfluidity) Macroscopicdynamic phenomena in superfluids (expansion, collective oscillations, moment of inertia) are described by theory of irrotational hydrodynamics More microscopic theories required to describe other superfluid phenomena (vortices, Landau critical velocity, pairing gap)

  3. HYDRODYNAMIC THEORY OF SUPERFLUIDS • Basic assumptions: • Irrotationality constraint • (follows from the phase of order parameter) • Conservation laws • (equation of continuity, equation for the current) Basic ingredient: - Equation of state

  4. Consequence of Galilean invariance: from the equation for the field operator to the hydrodynamic equations of superfluids Heisenberg equation for the field operator in uniform systems (Bose field) (similar equation for Fermi field operator) fluid at rest fluid moving with velocity v If is solution, is also solution (Galilean transformation with velocity v) Order parameter ( in Fermi case) aquires phase in Fermi case

  5. Gradient of the phase Superfluid velocity in Fermi case IRROTATIONALITY of flow is fundamental feature of superfluids: - quenching of moment of inertia - quantization of circulation and quantized vortices) Time derivative of the phase Relationship for superfluid velocity andequation for the phase are expected to hold also if order parameter varies slowly in space and time as well as in the presence of a smooth external potential.

  6. HYDRODYNAMIC EQUATIONS AT ZERO TEMPERATURE Hydrodynamic equations of superfluids (T=0) Closed equations for density and superfluid velocity field irrotationality

  7. KEY FEATURES OF HD EQUATIONS OF SUPERFLUIDS • Have classical form(do not depend on Planck constant) • Velocity field is irrotational • - Are equations for the total density (not for the condensate density) • Should be distinguished from rotational hydrodynamics. • - Applicable to low energy, macroscopic, phenomena • Hold for both Bose and Fermi superfluids • Depend on equation of state • (sensitive to quantum correlations, statistics, dimensionality, ...) • - Equilibrium solutions (v=0) consistent with LDA What do we mean by macroscopic, low energy phenomena ? size of Cooper pairs BEC superfluids BCS Fermi superfluids healing length more restrictive than in BEC superfluid gap

  8. WHAT ARE THE HYDRODYNAMIC EQUATIONS USEFUL FOR ? • They provide quantitative predictions for • Expansion of the gas follwowing sudden release of the trap • - Collective oscillations excited by modulating harmonic trap Quantities of highest interest from both theoretical and experimental point of view • Expansion provides information on • release energy, sensitive to anisotropy • Collective frequencies are measurable with highest precision • and can provide accurate test of equation of state

  9. Initially the gas is confined in anisotropic trap • in situ density profile is anisotropic too • What happens after release of the trap ? Expansion from anysotropic trap Non interacting gas expands isotropically • - For large times density distribution become isotropic • Consequence of isotropy of momentum distribution • holds for ideal Fermi gas and ideal Bose gas above • Ideal BEC gas expands anysotropically because • momentum distribution of condensate is anysotropic

  10. Superfluids expand anysotropically Hydrodynamic equations can be solved after switching off the external potential For polytropic equation of state (holding for unitary Fermi gas ( ) and in BEC gases ( )), and harmonic trapping, scaling solutions are available in the form (Castin and Dum 1996; Kagan et al. 1996) with the scaling factors satisfying the equation and - Expansion inverts deformation of density distribution, being faster in the direction of larger density gradients (radial direction in cigar traps) - expansion transforms cigar into pancake, and viceversa.

  11. Bosons Expansion of BEC gases ideal gas ideal gas HD HD Experiments probe HD nature of the expansion with high accuracy. Aspect ratio

  12. EXPANSION OF ULTRACOLD FERMI GAS Fermions Hydrodynamics predicts anisotropic expansion inFermi superfluids (Menotti et al,2002) HD theory First experimental evidence for hydrodynamic anisotropic expansion inultra cold Fermi gas (O’Hara et al, 2002) collisionless

  13. Fermions Measured aspect ratio after expansion along the BCS-BEC crossover of a Fermi gas (R. Grimm et al., 2007) prediction of HD at unitarity prediction of HD for BEC

  14. Fermions • - Expansion follows HD behavior • on BEC side of the resonance and at unitarity. • - on BCS side it behaves more and more like • in non interacting gas (asymptotic isotropy) • Explanation: • - on BCSside superfluid gap becomes soon • exponentially small during the expansion • and superfluidity is lost. • At unitarity gap instead always remains of the • order of Fermi energy and hence pairs are • not easily broken during the expansion

  15. Collective oscillations in trapped gases Collective oscillations: unique tool to explore consequence of superfluidity and test the equation of state of interacting quantum gases (both Bose and Fermi) Experimental data for collective frequencies are available with high precision

  16. Propagation of sound in trapped gases In uniform medium HD theory gives sound wave solution with In trapped gasessound waves can propagate if wave length is smaller than axial size of the condensate. Condition is easily satisfied in elongated condensates.

  17. Propagation of sound in elongated traps • If wave length is larger than radial size of • elongated trapped gas sound has 1D character • where and n is determined by TF eq. • one finds For BEC gas ( ) (Zaremba, 1998) (Capuzzi et al, 2006) For unitary Fermi gas ( )

  18. Bosons Sound wave packets propagating in a BEC (Mit 97) velocity of sound as a function of central density

  19. Fermions Sound wave packets propagating in an Interacting Fermi gas (Duke, 2006) behavior along the crossover BCS mean field QMC • Difference bewteen BCS and QMC reflects: • at unitarity: different value of in eq. of state • On BEC side different molecule-molecule scattering length

  20. Collective oscillations in harmonic trap When wavelength is of the order of the size of the atomic cloud sound is no longer a useful concept. Solve linearized 3D HD equations where is non uniform equilibrium Thomas Fermi profile Solutions of HD equations in harmonic trap predict both surface and compression modes (first investigated in dilute BEC gases (Stringari 96)

  21. Surface modes • Surface modes are unaffected by equation of state • For isotropic trap one finds where is angular momentum • surface mode is driven by external potential, not by surface tension • Dispersion law differs from ideal gas value (interactioneffect) Bosons Surface modes in BEC’s, Mit 2000 m=2 m=4

  22. Fermions l=2 Quadrupole mode measured on ultracold Fermi gas along the crossover (Altmeyer et al. 2007) Ideal gas value HD prediction Enhancement of damping Minimum damping near unitarity

  23. Fermions • - Experiments on collective oscillations show that • on the BCS side of the resonance superfluidity is • broken for relatively small values of • (where gap is of the order of radial oscillator frequency) • Deeper in BCS regime frequency takes • collisionless value • - Damping is minimum near resonance

  24. Compression modes • Sensitive to the equation of state • analytic solutions for collective frequencies available for polytropic equation of state • Example: radial compression mode in cigar trap • At unitarity ( ) one predicts universal value • For a BEC gas one finds m=0 radial compression exp: mode at T=0 (Ens 2001) theory: Bosons

  25. Fermions • Equation of state along BCS-BEC crossover • - Fixed Node Diffusion MC (Astrakharchick et al., 2004) • Comparison with mean field BCS theory ( - - - - - )

  26. Fermions Radial breathing mode at Innsbruck (Altmeyer et al., 2007) MC equation of state(Astrakharchick et al., 2005) includes beyond mf effects does not includes beyond mf effects BCS eq. of state (Hu et al., 2004) universal value at unitarity Measurement of collective frequencies provides accurate test of equation of state !!

  27. Fermions Main conclusions concerning the m=0 radial compression mode in superfluid Fermi gases • Accurate confirmation of the universal HD value • predicted at unitarity. • Accurate confirmation of QMC equation of state on the BEC side of • the resonance. • First evidence for Lee Huang Lee effect (enhancement of frequency • with respect to BEC value (role of quantum fluctuations) • LHY effect very sensitive to thermal effects (thermal fluctuations • prevail on quantum fluctuations except at very low temperature)

  28. Landau’s critical velocity While in BEC gas sound velocity provides critical velocity, in a Fermi BCS superfluid critical velocity is fixed by pair breaking mechanisms (role of the gap)

  29. Landau’s critical velocity Dispersion law of elementary excitations • - Landau’s criterion for superfluidity (metastability): • fluid moving with velocity smaller than critical velocity cannot decay • (persistent current) • - Ideal Bose gas and ideal Fermi gas one has • In interacting Fermi gas one predicts two limiting cases: BCS (role of the gap) BEC (Bogoliubov dispersion) (sound velocity)

  30. Fermions Dispersion law along BCS-BEC crossover BCS BEC gap gap gap unitarity BEC Critical velocity (Combescot, Kagan and Stringari 2006) Sound velocity B resonance Landau’s critical velocity is highest near unitarity !! BCS BEC

  31. Some conclusions • Order parameter: basic ingredient characterizing superfluid behavior • (consequence of long range order) • Microscopic theory available for dilute Bose gas (GP equation). • Approximate theories available for Fermi gases (ex: BdG equation) • Modulus of order parameter directly measurable in dilute Bose gas • (coincides with sqrt of density distribution at T=0). • In Fermi superfluid order parameter not easily experimentally accessible • (some information available through rf transition) • Phase of order parameter: basic ingredient for dynamic theory • of superfluids. • Systematic confirmation of superfluid dynamic behavior available from • the study of collective oscillations

  32. General reviews on BEC and Fermi superfluidity • - Theory of Bose-Einstein Condensation in trapped gases • F. Dalfovo et al., Rev. Mod. Phys. 71, 463 (1999) • Bose-Einstein Condensation in Dilute Gases • C. Pethick and H. Smith (Cambridge 2001) • - Bose-Einstein Condensation in the Alkali Gases: • Some Fundamental concepts • A. Leggett, Rev. Mod. Phys. 73, 333 (2001) • Bose-Einstein Condensation • L. Pitaevskii and S. Stringari (Oxford 2003 • Ultracold Atomic Fermi gases • Proceedings of 2006 Varenna Summer School • M. Inguscio, W. Ketterle, and Ch. Salomon (in press) • - Theory of Ultracold Fermi gases • S. Giorgini et al. cond-mat/0706.3360 (submitted to Rev.Mod.Phys.)

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